The energy spectra of TeV sources measured with the Durham Mark 6 Telescope

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dc.creatorChadwick, P. M.
dc.creatorLyons, K.
dc.creatorMcComb, T. J. L.
dc.creatorOrford, K. J.
dc.creatorOsborne, J. L.
dc.creatorRayner, S. M.
dc.creatorShaw, S. E.
dc.creatorTurver, K. E.
dc.date1999-06-08
dc.date.accessioned2026-07-07T02:31:55Z
dc.date.available2026-07-07T02:31:55Z
dc.descriptionA programme of detailed simulations of the response of the Durham Mark 6 atmospheric Cherenkov telescope is in progress. The effective collecting area for triggering by gamma-ray showers after application of selection criteria is derived as a function of energy. An initial result from the larger events in the 1996 and 1997 observations of the BL Lac PKS 2155-304 is that the time averaged flux above 1.5 TeV was (6.7 +/- 2.2) x 10^-8 m^-2 s^-1.
dc.description4 pages, 3 figures, to appear in the Proceedings of 26th International Cosmic Ray Conference (Salt Lake City, 1999)
dc.identifierhttps://arxiv.org/abs/astro-ph/9906138
dc.identifierhttp://arxiv.org/abs/astro-ph/9906138
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14326
dc.subjectAstrophysics
dc.titleThe energy spectra of TeV sources measured with the Durham Mark 6 Telescope
dc.typetext

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